Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum)

M. De Wilde; A.G.M. Pietrow; M.K. Druett; A. Pastor Yabar; J. Koza; I. Kontogiannis; O. Andriienko; A. Berlicki; A.R. Brunvoll; J. de la Cruz Rodríguez; J. Thoen Faber; R. Joshi; D. Kuridze; D. Nóbrega-Siverio; L.H.M. Rouppe van der Voort; J. Rybák; E. Scullion; A. M. Silva; Z. Vashalomidze; A. Vicente Arévalo; A. Wiśniewska; R. Yadav; T.V. Zaqarashvili; J. Zbinden; E. S. Øyre

doi:10.1051/0004-6361/202660990e

Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum)

M. De Wilde, A.G.M. Pietrow^*, M.K. Druett, A. Pastor Yabar, J. Koza, I. Kontogiannis, O. Andriienko, A. Berlicki, A.R. Brunvoll, J. de la Cruz Rodríguez, J. Thoen Faber, R. Joshi, D. Kuridze, D. Nóbrega-Siverio, L.H.M. Rouppe van der Voort, J. Rybák, E. Scullion, A. M. Silva, Z. Vashalomidze, A. Vicente ArévaloA. Wiśniewska, R. Yadav, T.V. Zaqarashvili, J. Zbinden, E. S. Øyre

^*Corresponding author for this work

School of Engineering Physics and Mathematics

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Abstract

Erratum for: A&A, 700, A275 (2025), https://doi.org/10.1051/0004-6361/202554870

Table 2 of our paper and the corresponding equation are inconsistent in their treatment of flare emission versus bolometric energy. The table values for the intercepts correspond to loge rather than log10 as stated in the equation. We provide the corrected table in this erratum.

Table 1.Correlation coefficients (R) and fitting parameters for the function log10(Cpeak) = b + alog10(E) corresponding to the data in Fig. 22 of the original paper.

Original language	English
Article number	C1
Number of pages	1
Journal	Astronomy and Astrophysics
Volume	710
DOIs	https://doi.org/10.1051/0004-6361/202660990e
Publication status	Published - 17 Jun 2026

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Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations
De Wilde, M., Pietrow, A. G. M., Druett, M. K., Yabar, A. P., Koza, J., Kontogiannis, I., Andriienko, O., Berlicki, A., Brunvoll, A. R., Rodríguez, J. D. L. C., Faber, J. T., Joshi, R., Kuridze, D., Nóbrega-Siverio, D., Voort, L. H. M. R. V. D., Rybák, J., Scullion, E., Silva, A. M., Vashalomidze, Z. & Arévalo, A. V. & 5 others, Wiśniewska, A., Yadav, R., Zaqarashvili, T. V., Zbinden, J. & Øyre, E. S., 1 Aug 2025, In: Astronomy and Astrophysics. 700, 21 p., A275.
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De Wilde, M., Pietrow, A. G. M., Druett, M. K., Pastor Yabar, A., Koza, J., Kontogiannis, I., Andriienko, O., Berlicki, A., Brunvoll, A. R., de la Cruz Rodríguez, J., Thoen Faber, J., Joshi, R., Kuridze, D., Nóbrega-Siverio, D., Rouppe van der Voort, L. H. M., Rybák, J., Scullion, E., Silva, A. M., Vashalomidze, Z., ... Øyre, E. S. (2026). Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum). Astronomy and Astrophysics, 710, Article C1. https://doi.org/10.1051/0004-6361/202660990e

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title = "Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum)",

abstract = "Erratum for: A\&A, 700, A275 (2025), https://doi.org/10.1051/0004-6361/202554870 Table 2 of our paper and the corresponding equation are inconsistent in their treatment of flare emission versus bolometric energy. The table values for the intercepts correspond to loge rather than log10 as stated in the equation. We provide the corrected table in this erratum. Table 1.Correlation coefficients (R) and fitting parameters for the function log10(Cpeak) = b + alog10(E) corresponding to the data in Fig. 22 of the original paper.",

author = "\{De Wilde\}, M. and A.G.M. Pietrow and M.K. Druett and \{Pastor Yabar\}, A. and J. Koza and I. Kontogiannis and O. Andriienko and A. Berlicki and A.R. Brunvoll and \{de la Cruz Rodr{\'i}guez\}, J. and \{Thoen Faber\}, J. and R. Joshi and D. Kuridze and D. N{\'o}brega-Siverio and \{Rouppe van der Voort\}, L.H.M. and J. Ryb{\'a}k and E. Scullion and Silva, \{A. M.\} and Z. Vashalomidze and \{Vicente Ar{\'e}valo\}, A. and A. Wi{\'s}niewska and R. Yadav and T.V. Zaqarashvili and J. Zbinden and {\O}yre, \{E. S.\}",

year = "2026",

month = jun,

day = "17",

doi = "10.1051/0004-6361/202660990e",

language = "English",

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De Wilde, M, Pietrow, AGM, Druett, MK, Pastor Yabar, A, Koza, J, Kontogiannis, I, Andriienko, O, Berlicki, A, Brunvoll, AR, de la Cruz Rodríguez, J, Thoen Faber, J, Joshi, R, Kuridze, D, Nóbrega-Siverio, D, Rouppe van der Voort, LHM, Rybák, J, Scullion, E, Silva, AM, Vashalomidze, Z, Vicente Arévalo, A, Wiśniewska, A, Yadav, R, Zaqarashvili, TV, Zbinden, J & Øyre, ES 2026, 'Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum)', Astronomy and Astrophysics, vol. 710, C1. https://doi.org/10.1051/0004-6361/202660990e

TY - JOUR

T1 - Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum)

AU - De Wilde, M.

AU - Pietrow, A.G.M.

AU - Druett, M.K.

AU - Pastor Yabar, A.

AU - Koza, J.

AU - Kontogiannis, I.

AU - Andriienko, O.

AU - Berlicki, A.

AU - Brunvoll, A.R.

AU - de la Cruz Rodríguez, J.

AU - Thoen Faber, J.

AU - Joshi, R.

AU - Kuridze, D.

AU - Nóbrega-Siverio, D.

AU - Rouppe van der Voort, L.H.M.

AU - Rybák, J.

AU - Scullion, E.

AU - Silva, A. M.

AU - Vashalomidze, Z.

AU - Vicente Arévalo, A.

AU - Wiśniewska, A.

AU - Yadav, R.

AU - Zaqarashvili, T.V.

AU - Zbinden, J.

AU - Øyre, E. S.

PY - 2026/6/17

Y1 - 2026/6/17

N2 - Erratum for: A&A, 700, A275 (2025), https://doi.org/10.1051/0004-6361/202554870 Table 2 of our paper and the corresponding equation are inconsistent in their treatment of flare emission versus bolometric energy. The table values for the intercepts correspond to loge rather than log10 as stated in the equation. We provide the corrected table in this erratum. Table 1.Correlation coefficients (R) and fitting parameters for the function log10(Cpeak) = b + alog10(E) corresponding to the data in Fig. 22 of the original paper.

AB - Erratum for: A&A, 700, A275 (2025), https://doi.org/10.1051/0004-6361/202554870 Table 2 of our paper and the corresponding equation are inconsistent in their treatment of flare emission versus bolometric energy. The table values for the intercepts correspond to loge rather than log10 as stated in the equation. We provide the corrected table in this erratum. Table 1.Correlation coefficients (R) and fitting parameters for the function log10(Cpeak) = b + alog10(E) corresponding to the data in Fig. 22 of the original paper.

U2 - 10.1051/0004-6361/202660990e

DO - 10.1051/0004-6361/202660990e

M3 - Comment/debate

SN - 0004-6361

VL - 710

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - C1

ER -

Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations (Corrigendum)

Abstract

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Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations

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